Short-term variability in the RS Canum Venaticorum system HR 1099

Details Short-term variability in the RS Canum Venaticorum system HR 1099 Short-term variability in the RS Canum Venaticorum system HR 1099

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103.1077b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Oct. 1991, p. 1077-1082.

Astronomy and Astrophysics

Astronomy

15

Binary Stars, G Stars, K Stars, Variable Stars, Absorption Spectra, Emission Spectra, Light Curve, Stellar Activity, Stellar Atmospheres, Stellar Models

Scientific paper

Observations of the RS CVn system HR 1099 made during the 1988 season are discussed. A dramatic reduction in extraphotospheric emission occurred on the primary during the observing period; this reduction is ascribed to the disappearance of a prominence on the K star. In addition, the system shows evidence for the process of mass transfer similar to those seen in the RS CVn system UX Ari.

Affiliated with

Also associated with

No associations

Rating

Short-term variability in the RS Canum Venaticorum system HR 1099 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Short-term variability in the RS Canum Venaticorum system HR 1099, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Short-term variability in the RS Canum Venaticorum system HR 1099 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1876757